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SPT-CL J0546-5345

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F. W. High; et al. (2010). "Optical Redshift and Richness Estimates for Galaxy Clusters Selected with the Sunyaev-Zel'dovich Effect from 2008 South Pole Telescope Observations".
45:, and optical telescopes allowed to identify cluster members and to measure the redshift. Using the velocity dispersion, the cluster mass has been estimated to 10 solar masses. 74:
M. Brodwin; et al. (2010). "SPT-CL J0546-5345: A Massive z>1 Galaxy Cluster Selected Via the Sunyaev-Zel'dovich Effect with the South Pole Telescope".
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is one of the most massive galaxy clusters ever found in the early universe. It is thought to be 7 billion light years away. It was discovered at the
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K. Vanderlinde; et al. (2010). "Galaxy Clusters Selected with the Sunyaev-Zel'dovich Effect from 2008 South Pole Telescope Observations".
379: 16: 234: 372: 42: 398: 34: 38: 235:"X-ray Properties of the First SZE-selected Galaxy Cluster Sample from the South Pole Telescope" 341: 408: 365: 353: 259: 199: 146: 93: 30: 8: 263: 203: 150: 97: 283: 249: 215: 211: 189: 162: 158: 136: 109: 83: 324: 271: 219: 166: 105: 54: 287: 113: 275: 267: 207: 154: 101: 403: 349: 314: 392: 279: 37:. The cluster has a redshift of z=1.067. Follow-up studies using the 254: 194: 141: 88: 20:
Wide-field view of the SPT-CL J0615-5746 galaxy cluster
390: 126: 373: 232: 120: 380: 366: 226: 179: 73: 253: 193: 140: 87: 67: 15: 391: 173: 336: 13: 233:K. Andersson; et al. (2011). 14: 420: 348:This galaxy-related article is a 340: 1: 60: 352:. You can help Knowledge by 319:2010 – 2011 212:10.1088/0004-637X/723/2/1736 159:10.1088/0004-637X/722/2/1180 7: 48: 10: 425: 335: 272:10.1088/0004-637X/738/1/48 106:10.1088/0004-637X/721/1/90 321: 308: 300: 242:The Astrophysical Journal 182:The Astrophysical Journal 129:The Astrophysical Journal 76:The Astrophysical Journal 35:Sunyaev-Zel'dovich-Effect 21: 19: 31:South Pole Telescope 312:distant (z~>=1) 264:2011ApJ...738...48A 204:2010ApJ...723.1736H 151:2010ApJ...722.1180V 98:2010ApJ...721...90B 22: 361: 360: 331: 330: 325:SPT-CL J2106-5844 322:Succeeded by 304:XMMU J2235.3-2557 55:SPT-CL J2106-5844 25:SPT-CL J0546-5345 416: 382: 375: 368: 344: 337: 301:Preceded by 298: 297: 292: 291: 257: 239: 230: 224: 223: 197: 188:(2): 1736–1747. 177: 171: 170: 144: 135:(2): 1180–1196. 124: 118: 117: 91: 71: 424: 423: 419: 418: 417: 415: 414: 413: 399:Galaxy clusters 389: 388: 387: 386: 333: 327: 318: 313: 311: 306: 296: 295: 237: 231: 227: 178: 174: 125: 121: 72: 68: 63: 51: 33:in 2008 by the 12: 11: 5: 422: 412: 411: 406: 401: 385: 384: 377: 370: 362: 359: 358: 345: 329: 328: 323: 320: 315:galaxy cluster 307: 302: 294: 293: 225: 172: 119: 65: 64: 62: 59: 58: 57: 50: 47: 9: 6: 4: 3: 2: 421: 410: 407: 405: 402: 400: 397: 396: 394: 383: 378: 376: 371: 369: 364: 363: 357: 355: 351: 346: 343: 339: 338: 334: 326: 317: 316: 310:Most massive 305: 299: 289: 285: 281: 277: 273: 269: 265: 261: 256: 251: 247: 243: 236: 229: 221: 217: 213: 209: 205: 201: 196: 191: 187: 183: 176: 168: 164: 160: 156: 152: 148: 143: 138: 134: 130: 123: 115: 111: 107: 103: 99: 95: 90: 85: 81: 77: 70: 66: 56: 53: 52: 46: 44: 40: 36: 32: 27: 26: 18: 409:Galaxy stubs 354:expanding it 347: 332: 309: 280:1721.1/96774 245: 241: 228: 185: 181: 175: 132: 128: 122: 82:(1): 90–97. 79: 75: 69: 28: 24: 23: 393:Categories 61:References 255:1006.3068 248:(1): 48. 220:119189086 195:1003.0005 167:119206180 142:1003.0003 89:1006.5639 288:31168807 114:54988474 49:See also 260:Bibcode 200:Bibcode 147:Bibcode 94:Bibcode 43:Chandra 39:Spitzer 404:Pictor 286:  218:  165:  112:  284:S2CID 250:arXiv 238:(PDF) 216:S2CID 190:arXiv 163:S2CID 137:arXiv 110:S2CID 84:arXiv 350:stub 276:hdl 268:doi 246:738 208:doi 186:723 155:doi 133:722 102:doi 80:721 395:: 282:. 274:. 266:. 258:. 244:. 240:. 214:. 206:. 198:. 184:. 161:. 153:. 145:. 131:. 108:. 100:. 92:. 78:. 41:, 381:e 374:t 367:v 356:. 290:. 278:: 270:: 262:: 252:: 222:. 210:: 202:: 192:: 169:. 157:: 149:: 139:: 116:. 104:: 96:: 86::

Index

Wide-field view of the SPT-CL J0615-5746 galaxy cluster
South Pole Telescope
Sunyaev-Zel'dovich-Effect
Spitzer
Chandra
SPT-CL J2106-5844
arXiv
1006.5639
Bibcode
2010ApJ...721...90B
doi
10.1088/0004-637X/721/1/90
S2CID
54988474
arXiv
1003.0003
Bibcode
2010ApJ...722.1180V
doi
10.1088/0004-637X/722/2/1180
S2CID
119206180
arXiv
1003.0005
Bibcode
2010ApJ...723.1736H
doi
10.1088/0004-637X/723/2/1736
S2CID
119189086

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